Very high energy observations of gamma-ray burst locations with the whipple telescope

D. Horan; R. W. Atkins; H. M. Badran; G. Blaylock; S. M. Bradbury; J. H. Buckley; K. L. Byrum; O. Celik; Y. C.K. Chow; P. Cogan; W. Cui; M. K. Daniel; I. De La Calle Perez; C. Dowdall; A. D. Falcone; D. J. Fegan; S. J. Fegan; J. P. Finley; P. Fortin; L. F. Fortson; G. H. Gillanders; J. Grube; K. J. Gutierrez; J. Hall; D. Hanna; J. Holder; S. B. Hughes; T. B. Humensky; G. E. Kenny; M. Kertzman; D. B. Kieda; J. Kildea; H. Krawczynski; F. Krennrich; M. J. Lang; S. LeBohec; G. Maier; P. Moriarty; T. Nagai; R. A. Ong; J. S. Perkins; D. Petry; J. Quinn; M. Quinn; K. Ragan; P. T. Reynolds; H. J. Rose; M. Schroedter; G. H. Sembroski; D. Steele; S. P. Swordy; J. A. Toner; L. Valcarcel; V. V. Vassiliev; R. G. Wagner; S. P. Wakely; T. C. Weekes; R. J. White; D. A. Williams

doi:10.1086/509567

Very high energy observations of gamma-ray burst locations with the whipple telescope

D. Horan, R. W. Atkins, H. M. Badran, G. Blaylock, S. M. Bradbury, J. H. Buckley, K. L. Byrum, O. Celik, Y. C.K. Chow, P. Cogan, W. Cui, M. K. Daniel, I. De La Calle Perez, C. Dowdall, A. D. Falcone, D. J. Fegan, S. J. Fegan, J. P. Finley, P. Fortin, L. F. FortsonG. H. Gillanders, J. Grube, K. J. Gutierrez, J. Hall, D. Hanna, J. Holder, S. B. Hughes, T. B. Humensky, G. E. Kenny, M. Kertzman, D. B. Kieda, J. Kildea, H. Krawczynski, F. Krennrich, M. J. Lang, S. LeBohec, G. Maier, P. Moriarty, T. Nagai, R. A. Ong, J. S. Perkins, D. Petry, J. Quinn, M. Quinn, K. Ragan, P. T. Reynolds, H. J. Rose, M. Schroedter, G. H. Sembroski, D. Steele, S. P. Swordy, J. A. Toner, L. Valcarcel, V. V. Vassiliev, R. G. Wagner, S. P. Wakely, T. C. Weekes, R. J. White, D. A. Williams

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Abstract

Gamma-ray burst (GRB) observations at very high energies ( VHE; E > 100 GeV) can impose tight constraints on some GRB emission models. Many GRB afterglow models predict a VHE component similar to that seen in blazars and plerions, in which the GRB spectral energy distribution has a double-peaked shape extending into the VHE regime. VHE emission coincident with delayed X-ray flare emission has also been predicted. GRB follow-up observations have had high priority in the observing program at the Whipple 10m gamma-ray telescope, and GRBs will continue to be high-priority targets as the next-generation observatory, VERITAS, comes online. Upper limits on the VHE emission at late times (>∼4 hr) from seven GRBs observed with the Whipple Telescope are reported here.

Original language	English (US)
Pages (from-to)	396-405
Number of pages	10
Journal	Astrophysical Journal
Volume	655
Issue number	1 I
DOIs	https://doi.org/10.1086/509567
State	Published - Jan 20 2007

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

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10.1086/509567

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Horan, D., Atkins, R. W., Badran, H. M., Blaylock, G., Bradbury, S. M., Buckley, J. H., Byrum, K. L., Celik, O., Chow, Y. C. K., Cogan, P., Cui, W., Daniel, M. K., De La Calle Perez, I., Dowdall, C., Falcone, A. D., Fegan, D. J., Fegan, S. J., Finley, J. P., Fortin, P., ... Williams, D. A. (2007). Very high energy observations of gamma-ray burst locations with the whipple telescope. Astrophysical Journal, 655(1 I), 396-405. https://doi.org/10.1086/509567

@article{9e5997a0df4c46338dc520c71b212644,

title = "Very high energy observations of gamma-ray burst locations with the whipple telescope",

abstract = "Gamma-ray burst (GRB) observations at very high energies ( VHE; E > 100 GeV) can impose tight constraints on some GRB emission models. Many GRB afterglow models predict a VHE component similar to that seen in blazars and plerions, in which the GRB spectral energy distribution has a double-peaked shape extending into the VHE regime. VHE emission coincident with delayed X-ray flare emission has also been predicted. GRB follow-up observations have had high priority in the observing program at the Whipple 10m gamma-ray telescope, and GRBs will continue to be high-priority targets as the next-generation observatory, VERITAS, comes online. Upper limits on the VHE emission at late times (>∼4 hr) from seven GRBs observed with the Whipple Telescope are reported here.",

author = "D. Horan and Atkins, {R. W.} and Badran, {H. M.} and G. Blaylock and Bradbury, {S. M.} and Buckley, {J. H.} and Byrum, {K. L.} and O. Celik and Chow, {Y. C.K.} and P. Cogan and W. Cui and Daniel, {M. K.} and {De La Calle Perez}, I. and C. Dowdall and Falcone, {A. D.} and Fegan, {D. J.} and Fegan, {S. J.} and Finley, {J. P.} and P. Fortin and Fortson, {L. F.} and Gillanders, {G. H.} and J. Grube and Gutierrez, {K. J.} and J. Hall and D. Hanna and J. Holder and Hughes, {S. B.} and Humensky, {T. B.} and Kenny, {G. E.} and M. Kertzman and Kieda, {D. B.} and J. Kildea and H. Krawczynski and F. Krennrich and Lang, {M. J.} and S. LeBohec and G. Maier and P. Moriarty and T. Nagai and Ong, {R. A.} and Perkins, {J. S.} and D. Petry and J. Quinn and M. Quinn and K. Ragan and Reynolds, {P. T.} and Rose, {H. J.} and M. Schroedter and Sembroski, {G. H.} and D. Steele and Swordy, {S. P.} and Toner, {J. A.} and L. Valcarcel and Vassiliev, {V. V.} and Wagner, {R. G.} and Wakely, {S. P.} and Weekes, {T. C.} and White, {R. J.} and Williams, {D. A.}",

year = "2007",

month = jan,

day = "20",

doi = "10.1086/509567",

language = "English (US)",

volume = "655",

pages = "396--405",

journal = "Astrophysical Journal",

issn = "0004-637X",

publisher = "American Astronomical Society",

number = "1 I",

}

Horan, D, Atkins, RW, Badran, HM, Blaylock, G, Bradbury, SM, Buckley, JH, Byrum, KL, Celik, O, Chow, YCK, Cogan, P, Cui, W, Daniel, MK, De La Calle Perez, I, Dowdall, C, Falcone, AD, Fegan, DJ, Fegan, SJ, Finley, JP, Fortin, P, Fortson, LF, Gillanders, GH, Grube, J, Gutierrez, KJ, Hall, J, Hanna, D, Holder, J, Hughes, SB, Humensky, TB, Kenny, GE, Kertzman, M, Kieda, DB, Kildea, J, Krawczynski, H, Krennrich, F, Lang, MJ, LeBohec, S, Maier, G, Moriarty, P, Nagai, T, Ong, RA, Perkins, JS, Petry, D, Quinn, J, Quinn, M, Ragan, K, Reynolds, PT, Rose, HJ, Schroedter, M, Sembroski, GH, Steele, D, Swordy, SP, Toner, JA, Valcarcel, L, Vassiliev, VV, Wagner, RG, Wakely, SP, Weekes, TC, White, RJ & Williams, DA 2007, 'Very high energy observations of gamma-ray burst locations with the whipple telescope', Astrophysical Journal, vol. 655, no. 1 I, pp. 396-405. https://doi.org/10.1086/509567

TY - JOUR

T1 - Very high energy observations of gamma-ray burst locations with the whipple telescope

AU - Horan, D.

AU - Atkins, R. W.

AU - Badran, H. M.

AU - Blaylock, G.

AU - Bradbury, S. M.

AU - Buckley, J. H.

AU - Byrum, K. L.

AU - Celik, O.

AU - Chow, Y. C.K.

AU - Cogan, P.

AU - Cui, W.

AU - Daniel, M. K.

AU - De La Calle Perez, I.

AU - Dowdall, C.

AU - Falcone, A. D.

AU - Fegan, D. J.

AU - Fegan, S. J.

AU - Finley, J. P.

AU - Fortin, P.

AU - Fortson, L. F.

AU - Gillanders, G. H.

AU - Grube, J.

AU - Gutierrez, K. J.

AU - Hall, J.

AU - Hanna, D.

AU - Holder, J.

AU - Hughes, S. B.

AU - Humensky, T. B.

AU - Kenny, G. E.

AU - Kertzman, M.

AU - Kieda, D. B.

AU - Kildea, J.

AU - Krawczynski, H.

AU - Krennrich, F.

AU - Lang, M. J.

AU - LeBohec, S.

AU - Maier, G.

AU - Moriarty, P.

AU - Nagai, T.

AU - Ong, R. A.

AU - Perkins, J. S.

AU - Petry, D.

AU - Quinn, J.

AU - Quinn, M.

AU - Ragan, K.

AU - Reynolds, P. T.

AU - Rose, H. J.

AU - Schroedter, M.

AU - Sembroski, G. H.

AU - Steele, D.

AU - Swordy, S. P.

AU - Toner, J. A.

AU - Valcarcel, L.

AU - Vassiliev, V. V.

AU - Wagner, R. G.

AU - Wakely, S. P.

AU - Weekes, T. C.

AU - White, R. J.

AU - Williams, D. A.

PY - 2007/1/20

Y1 - 2007/1/20

N2 - Gamma-ray burst (GRB) observations at very high energies ( VHE; E > 100 GeV) can impose tight constraints on some GRB emission models. Many GRB afterglow models predict a VHE component similar to that seen in blazars and plerions, in which the GRB spectral energy distribution has a double-peaked shape extending into the VHE regime. VHE emission coincident with delayed X-ray flare emission has also been predicted. GRB follow-up observations have had high priority in the observing program at the Whipple 10m gamma-ray telescope, and GRBs will continue to be high-priority targets as the next-generation observatory, VERITAS, comes online. Upper limits on the VHE emission at late times (>∼4 hr) from seven GRBs observed with the Whipple Telescope are reported here.

AB - Gamma-ray burst (GRB) observations at very high energies ( VHE; E > 100 GeV) can impose tight constraints on some GRB emission models. Many GRB afterglow models predict a VHE component similar to that seen in blazars and plerions, in which the GRB spectral energy distribution has a double-peaked shape extending into the VHE regime. VHE emission coincident with delayed X-ray flare emission has also been predicted. GRB follow-up observations have had high priority in the observing program at the Whipple 10m gamma-ray telescope, and GRBs will continue to be high-priority targets as the next-generation observatory, VERITAS, comes online. Upper limits on the VHE emission at late times (>∼4 hr) from seven GRBs observed with the Whipple Telescope are reported here.

UR - http://www.scopus.com/inward/record.url?scp=33846871689&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=33846871689&partnerID=8YFLogxK

U2 - 10.1086/509567

DO - 10.1086/509567

M3 - Article

AN - SCOPUS:33846871689

SN - 0004-637X

VL - 655

SP - 396

EP - 405

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 1 I

ER -

Very high energy observations of gamma-ray burst locations with the whipple telescope

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